Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z ∼ 3

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Volume 696 (April 2025)

A&A, 696 (2025) A95

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Table 4.

QSO-galaxies cross-correlation and galaxy-galaxy auto-correlation lengths.

Correlation	r₀ (h⁻¹ cMpc)	r₀ (h⁻¹ cMpc)	γ
function	\|Δv\|≤1000 km s⁻¹	\|Δv\|≤1500 km s⁻¹
$w_{QG}^{MQN 01}$ $w_{\mathrm{QG}}^{\mathrm{MQN01}}$	$23 . 06_{- 3.43}^{+ 3.49}$ $23.06^{+3.49}_{-3.43}$	$22 . 39_{- 3.36}^{+ 3.72}$ $22.39^{+3.72}_{-3.36}$	1.5
	$15 . 71_{- 1.83}^{+ 1.79}$ $15.71^{+1.79}_{-1.83}$	$14 . 08_{- 2.01}^{+ 1.76}$ $14.08^{+1.76}_{-2.01}$	1.8

$w_{GG}^{UDF}$ $w_{\mathrm{GG}}^{\mathrm{UDF}}$	$4 . 25_{- 1.44}^{+ 1.56}$ $4.25^{+1.56}_{-1.44}$	$2 . 65_{- 1.10}^{+ 1.28}$ $2.65^{+1.28}_{-1.10}$	1.5
	$3 . 54_{- 1.08}^{+ 1.05}$ $3.54^{+1.05}_{-1.08}$	$2 . 36_{- 0.83}^{+ 0.92}$ $2.36^{+0.92}_{-0.83}$	1.8

Notes. The correlation lengths are derived by fitting Eq. (10) from TS12 to the correlation functions measured for the MUSE spectroscopic sample and the field galaxies identified in the UDF-MOSAIC (Bacon et al. 2023), respectively.

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